Plaattektoniek en Mickey Mouse: de bewegingen van de Aarde en de geologie van Marokko. G. Bertotti - TUDelft
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1 Plaattektoniek en Mickey Mouse: de bewegingen van de Aarde en de geologie van Marokko G. Bertotti - TUDelft
2 Moving continents Continent with matching boundaries Same fauna in different continents Similar rocks in unexpected places
3 Moving continents Very accurate displacement vectors Rigid plates with mobile margins Oceanic ridges Subduction zones Transform zones
4 how does it function?
5 The motor A simple kinematics; simple physics No changes Oceanic crust is created at ridges Oceanic crust is eliminated at subduction zones
6 Mickey Mouse In reality Something does not work
7 Evidence #1: the birth of rifts The East African rift A new plate boundary is being formed
8 Continental rifts and passive continental margins b) 0 depth (k m) Neogene Paleogene Cretaceous Jurassic 200 Middle - Upper Triassic?Devonian - Lower Triassic Basement Moho?? High velocity body (+8 km/s) In tra man tle reflections distance (km) 50 the North Sea 0 Moho If extension continues, break-up occurs and two passive continental margins are formed
9 Evidence #2: end of convergence, birth of a mountain belt Continent-continent collision
10 Continent-continent collision No way Mickey Mouse can do this Change in plate kinematics is needed
11 Continent-continent collision
12 Mickey-Mouse plate tectonics Fails to explain major features Major advance in knowledge during the last years 1) Tomography 2) Numerical modelling of mantle processes
13 tomography Deviations from an assumed velocity model are measured Assuming that waves are travelling through a homogeneous medium then velocity changes are controlled by temperature
14 Physically speaking, not obvious: rocks keep their temperature (difference) for a very long time The case of subduction zones Courtesy of T. Becker
15 Tomography: extension and subduction Western Europe Japan
16 Detailed subduction Japan more at depth With more detail The 650km discontinuity
17 The 650km discontinuity Spinel changes to perovskite, with a 10% increase in density and corresponding increase in seismic velocities olivine spinel perovskite It forms a strong barrier to further subduction and makes less constant something which is constant at the surface
18 Going deeper A fairly simple picture at depth
19 Going at 2800km depth Xiang Li & Zhong 2010
20 Mantle structure Complex uppermost 700km Simple structure beneath 700km with two superplumes separated by areas of descending mantle How do they interact? Faccenna et al., 2012
21 Modelling mantle convection Courtesy of S. Zhong downward moving upward moving Huge progress in the very difficult field of mantle convection
22 Deep and shallow 75Myr 125Myr 155Myr 183Myr 198Myr 232Myr
23 Xiang Li & Zhong Ma ciclicity
24 New plate tectonics A multiscale process with large wavelength, mantle driven processes, interacting and disrupting shorter wavelengths, lithosphere driven phenomena
25 Creating mountains and sedimentary basins Isostasy, the law of floating bodies H z ρ 2 ρ 1 h 1 ( h 1 h H = H ) ρ = ρ h ( ρ2 ρ1) ρ 1
26 density root (km) height (km) 2, , ,
27 Isostasy works very well But not everywhere: dynamic topography
28 Dynamic topography Too low Too high dynamic contribution (slab) dynamic contribution isostasy isostasy actual topography actual topography Faccenna
29 Dynamic topography The place to look for: Africa, especially its southern part (too) high elevations, very large wavelength
30 Dynamic topography High mountains, strong erosion Good for Namibia!
31 Morocco Something on our work on Morocco Great country with beautiful geology
32 A classic Atlantic-type continental margin oceanic crust born 175 Ma: after 175Ma, passive margin stage
33 Upper Cretaceous shallow marine (post-extension) Paleozoic + isolated Triassic patches (pre-extension) A well-behaved margin?
34 Low-temperature geochronology Fission 238 U creates tracks which are annealed when temperatures are above 120⁰ and accumulate when temperatures are lower 30µm Dating the moment when rocks cooled below a given temperature (= became shallower than 2-3km)
35 Low-temperature geochronology
36 Surprises come! Upper Cretaceous shallow marine Ghorbal et al., 2008 Paleozoic + isolated Triassic patches 131±9/147±7 117±8/146±11 Rocks move upward during the passive continental stage
37 A domain with strong exhumation Flanked by one with strong subsidence 1100km
38 The applied side
39 A widespread phenomenon The Pandora box stage
40 Conclusions? An exciting planet!
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